Sycorax (moon) Saturday, June 20, 2009


Sycorax
Discovery
Discovered by Philip D. Nicholson,
Brett J. Gladman,
Joseph A. Burns,
John J. Kavelaars
using the Hale telescope
Discovered in September 6, 1997
Orbital characteristics
Mean radius 12,179,000 km
Eccentricity 0.5224[1]
Orbital period 1288.28 d
Inclination 159° (to the ecliptic)[2]
Is a satellite of Uranus
Physical characteristics
Mean diameter ~150 km (estimate)[2][3]
Surface area ~70,000 km² (estimate)
Volume ~1,800,000 km³ (estimate)
Mass ~2.3 × 1018 kg (estimate)
Mean density ~1.3 g/cm³ (assumed)
Surface gravity ~0.040 m/s2 (estimate)
Escape velocity ~0.064 km/s (estimate)
Rotation period ?
Axial tilt
Albedo 0.04 (assumed)[2][3]
Surface temp.
min mean max

~64 K (estimate)
Atmospheric pressure 0 kPa

Sycorax (pronounced /ˈsɪkɵræks/ SIK-or-aks) is the largest retrograde irregular satellite of Uranus. Sycorax was discovered on 1997-09-06 by Brett J. Gladman, Philip D. Nicholson, Joseph A. Burns, and John J. Kavelaars using the 200-inch Hale telescope, together with Caliban and given the temporary designation S/1997 U 2.[4]

Officially confirmed as Uranus XVII, it was named after Sycorax, Caliban's mother in William Shakespeare's play The Tempest.

Orbit

Retrograde irregular satellites of Uranus.

Sycorax follows a distant orbit, more than 20 times further from Uranus than the furthest regular moon Oberon. Its orbit is retrograde, moderately inclined and eccentric. The orbital parameters suggest that it may belong, together with Setebos and Prospero, to the same dynamic cluster, suggesting common origin.[5] The diagram illustrates the orbital parameters of the retrograde irregular satellites of Uranus (in polar co-ordinates) with the eccentricity of the orbits represented by the segments extending from the pericentre to the apocentre.

Physical characteristics

The diameter of Sycorax is estimated at 150 km (assuming albedo of 0.04)[2][3] making it the largest irregular satellite of Uranus, comparable in size with Himalia, the biggest irregular satellite of Jupiter.

The satellite appears light-red (colour indices B-V=0.87 V-R=0.44,[6] B-V=1.01 V-R=0.48[7]) redder than Himalia but still less red than most Kuiper Belt Objects.

The rotation period could not be estimated conclusively (best fit ~4 h).[7]

See also

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